Pith Number
pith:YJGS5GQR
pith:2015:YJGS5GQR3ABPDFD4ZCMPUQRJ7R
not attested
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not stored
refs pending
Capabilities of future intensity interferometers for observing fast-rotating stars: imaging with two- and three-telescope correlations
arxiv:1507.07635 v1 · 2015-07-28 · astro-ph.IM
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YJGS5GQR3ABPDFD4ZCMPUQRJ7R}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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4
Citations
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Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-05-18T01:33:42.094139Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c24d2e9a11d802f1947cc898fa4229fc7ca2a178cd080dabdb8a486d6f1f0b4f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YJGS5GQR3ABPDFD4ZCMPUQRJ7R \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: c24d2e9a11d802f1947cc898fa4229fc7ca2a178cd080dabdb8a486d6f1f0b4f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e6da421f22e2264d7da6384f01197ad93e7bb7bf9d0e7d08161cbc4b00ba6880",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.IM",
"submitted_at": "2015-07-28T03:50:45Z",
"title_canon_sha256": "6481d8d970bd0cb640837d98d14747cc4f082ea4fa2335b1ec15f4a1e32e86dc"
},
"schema_version": "1.0",
"source": {
"id": "1507.07635",
"kind": "arxiv",
"version": 1
}
}